Wednesday, March 20, 2013

Solution To The Third Test Queston Of The Last Test Of Course 11

The angular momentum eigenstates of corelative Planck-like phenomena that are adjacent and are also of different universes bear a different wobble than a covariant, codeterminable, codifferential relativistic oscillation of ~1.104735878*10^(-81)I degrees are not necessarily in a physically Laplacian-based mapped-out condition that is norm when comparing their relative distributions that these bear relative to one another during BRST.  Yet, their mentioned relativistic wobble that these PLP bear relative to one another is orphoganal, or norm, with a wobble that has a scalar amplitude that is off from the said ~1.104735878*10^(-81)I degrees as is according to the angling that the various given arbitary PLP that are here from different universes are off of a completely norm-state condition -- off from being orphoganal to one another.  This is because the wobbling of angular momentum indices of PLP work to bear a wobble that works to forma covariant, codifferentiable, and codeterminable condition of normalcy when the directly related mini-string segments torque -- the said torque of which happens in such a manner that it is delineated from different PLP that interact in a manner that is due to the condition that all touch and coupling involves a 90 degree interaction.  Thie causes a Dirac of Clifford Expansion in the corelative wobble that therefore makes the corelative vibrations of wobble work to touch in an orphoganal manner that is here off from ~1.104735878*10^(-81)I degrees as is according to how off of normalcy that the correspondingly different PLP are off from normal -- as is according to how these are to be mapped out -- via an extrapolation of their Laplacian-based settings over a course of an iteration of group BRST during group instanton.  As one extrapolates Planck-like phenomena-related characteristics that are apart from adjacency, one is to make a Laplacian-based mapping that is based upon the mapping as to what would be the proper orientation of orphoganation -- as is according to the right-hand-rule for up to 32 dimensions at what would be here a 90 degree relativistic corelation.  This works to re-establish basic norm-related conditons for each succeeding layer of adjacency for up to  32piI degrees that then restarts at 0 degrees, once one goes out 64 layers out from the initial adjacent layer that we are considering in this given arbitrary case.  Depending on how off of norm the physical placement of teh corelative PLP aare physically mapped, relative to one another -- when given a Laplacian-based extrapolation, the said vibratorial oscillations of the directly related angular momentum eigenstates will be norm with a wobble that is variant from ~1.104735878*10^(-81)I degrees, just as the physical placement of their corelative PLP is off from 90 degrees.  The said levels of adjacency just mentioned here are not specifically bearing on the conditions of relative proximity.
I hope that you are checking your solutions!
Sincerely, Samuel David Roach.

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